Sun's Path and Altitude Concepts

Sun's Path and Altitude Concepts

Assessment

Interactive Video

Geography

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video tutorial by Mr. Rabbit explains the sun's path lab, focusing on calculating the altitude of the noon sun at different Earth locations. It covers equinoxes, solstices, and the sun's vertical ray, providing a step-by-step guide to plotting the sun's path and understanding seasonal changes. The tutorial also includes instructions for labeling Polaris and offers additional resources for further study.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main focus of the Sun's Path Lab?

Measuring the distance to the Sun

Studying the phases of the Moon

Calculating the altitude of the noon Sun

Calculating the Earth's rotation speed

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Where is the Sun's vertical ray located during an equinox?

At the Tropic of Cancer

At the Tropic of Capricorn

At the equator

At the Arctic Circle

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

On June 21st, where is the Sun's vertical ray located?

At the North Pole

At 23.5 degrees south

At 23.5 degrees north

At the equator

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How do you calculate the noon Sun's altitude for the equinoxes?

Add 23.5 degrees to the latitude

Subtract the latitude from 90 degrees

Multiply the latitude by 2

Divide the latitude by 2

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to the noon Sun's altitude during the winter solstice at 66.5 degrees north?

It decreases to zero degrees

It remains the same

It increases by 23.5 degrees

It becomes negative

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the angle of the noon Sun during the summer solstice at 66.5 degrees north?

90 degrees

66.5 degrees

47 degrees

23.5 degrees

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the position of Polaris relative to the observer's latitude?

It is at the North Pole

It is at the equator

It equals the observer's latitude

It is always at 90 degrees

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